Everything Worth Knowing About ... the Dark Universe

See the light on dark matter and dark energy.

By Adam Hadhazy|Monday, June 12, 2017
RELATED TAGS: COSMOLOGY
dark-universe-cover
dark-universe-cover
NASA/ESA/S. Beckwith (STScI)/The Hubble Heritage Team (STScI/AURA)

Say the universe is a restaurant entrée. Astonishingly, everything that we can discern on the plate, so to speak — protons, paramecia, people, planets, pulsars, you name it — altogether adds up to a mere sprig of parsley. To a cosmic garnish such as ourselves, the vast majority of the universe is invisible, an empty plate dominated by “dark” matter and a “dark” energy. The effects of these phenomena are writ large in space, yet their true natures have frustratingly evaded every instrument we’ve brought to bear.


DARK MATTER

gravitational-lensing
gravitational-lensing
Gravitational lensing
NASA/ESA/Judy Schmidt

How Do We Know It’s There?

  • The cosmos would fling itself apart were it not for a gravitational glue provided by tremendous, yet unseen, amounts of mass. Factoring in all the ordinary matter we cannot see — contained in exoplanets, galactic gas clouds, and black holes, none of which emit light — still isn’t enough to make up the difference.
  • The immense gravity from clusters of galaxies warps the light coming from more distant objects, acting like a cosmic magnifying glass. This gravitational lensing is far too strong to be caused by plain ol’ matter.
  • Gas filaments (in orange at right) connect scattered groups of galaxies. This vast cosmic web makes structural sense only when explained by underlying concentrations of dark matter (blue).
  • Ordinary matter also can’t explain temperature fluctuations in the Big Bang’s relic afterglow. Known as the cosmic microwave background (CMB), it’s visible everywhere in the sky as microwaves.
cosmic-structure
cosmic-structure
Cosmic structure
ESO/Illustris Collaboration
What Could It Be?

Probably an elusive kind of subatomic particle (or particles) that outnumbers normal matter particles by 5 to 1. The two leading contenders:

  • WIMPs: Cute acronym for weakly interacting massive particles, much heavier than the familiar protons and neutrons in atomic nuclei. WIMPs would “feel” matter through gravity and the so-called weak force, which is responsible for why atoms radioactively decay.
  • Axions: A two-for-one special? Physicists originally cooked up the axion to explain why neutrons don’t spin in electric fields. The particle’s attendant properties — insanely low-mass, mostly indifferent to matter and highly abundant — neatly check off many dark matter boxes, too.
CMB
CMB
CMB
ESA/The Planck Collaboration

How Do We Look for It?

Typically, dark matter aloofly passes through Earth, but in rare instances it might interact with normal matter; the trick is to tell when. Experiments like SuperCDMS and LUX-ZEPLIN rely on metal germanium crystals and liquid xenon, respectively, as their dark matter finders. Come 2020, these experiments will run in deep underground mines, shielded from the cosmic radiation striking our planet’s surface. The Axion Dark Matter eXperiment, started at Lawrence Livermore National Laboratory before moving to the University of Washington, seeks the subtle signatures — just a trillionth of a trillionth of a watt — left by axions as they’re snagged by a strong magnetic field. Telescopes are also on the lookout for telltale gamma rays from space, in case dark matter commits the particle version of suicide and self-destructs.


DARK ENERGY

How Do We Know It’s There?

Space telescopes studying the Big Bang’s relic radiation (the cosmic microwave background) have found the universe is almost perfectly flat. That means light travels in straight lines unless it encounters mass. Scientists say this only really makes sense in a universe brimming with some kind of dark energy.

Dark energy would also explain why our universe’s expansion is accelerating. Although we’ve known for about a century that galaxies are receding from ours, scientists long speculated that matter’s gravitational heft would eventually slow cosmic expansion — maybe even reverse it, culminating in what’s called a Big Crunch. In 1998, however, astonished astronomers discovered the opposite. A certain kind of exploding star, called a supernova, turned out to be fainter than expected in the distant past, indicating that the universe is ballooning at an ever-faster rate, and has been for nearly half of its 13.8 billion-year existence. At the current clip of cosmic growth, the distance between galaxies will double in 10 billion years.

Roen Kelly/Discover
What Could It Be?

Many astrophysicists wager that dark energy is inherent to the empty vacuum of space, comprising the universe’s bulk by virtue of being near-ubiquitous. After all, there’s a lot of emptiness out there.

How Do We Look for It?

Huge sky surveys measuring the distribution of billions of galaxies over cosmic history could offer clues about the evolution of dark energy, as well as its enigmatic properties. Key missions include NASA’s Wide Field Infrared Survey Telescope (WFIRST) and the European Space Agency’s Euclid space telescope, plus the ground-based Large Synoptic Survey Telescope, opening in Chile in the 2020s.


DISCLAIMER

composition-of-universe
composition-of-universe
NASA
Could Dark Matter and Dark Energy Be Wrong?

Oh yeah, big time. It could be that neither dark matter nor dark energy exists. Sure, it would require a major rejiggering of Albert Einstein’s extremely well-tested theories: Gravity would somehow have to operate differently on epic, cosmic scales. But don’t count out the possibility that current ideas about the universe are totally wrong. Many scientists freely admit they’re really — ahem — in the dark about the dark universe.

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